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English: The image shows the vertical structure of the atmosphere of Jupiter. The temperature is shown as a function of pressure (black line). The approximate altitudes of atmospheric transitions troposphere–stratosphere (tropopause) and stratosphere–thermosphere are shown, as well as tropospheric cloud layers. The information was taken from
Seiff, Alvin; Kirk, Don B.; Knight, Tony C.D. et.al. (1998). "Thermal structure of Jupiter's atmosphere near the edge of a 5-μm hot spot in the north equatorial belt". Journal of Geophysical Research 103: 22,857–22,889. DOI:10.1029/98JE01766.
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I, the copyright holder of this work, hereby publish it under the following licenses:
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GNU head Permission is granted to copy, distribute and/or modify this document under the terms of the GNU Free Documentation License, Version 1.2 or any later version published by the Free Software Foundation; with no Invariant Sections, no Front-Cover Texts, and no Back-Cover Texts. A copy of the license is included in the section entitled GNU Free Documentation License.
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5 October 2008

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Date/TimeThumbnailDimensionsUserComment
current05:53, 1 February 2012Thumbnail for version as of 05:53, 1 February 20123,000 × 1,934 (56 KB)Bewareircdchanged unit from mbar (traditional european unit) to Pa (pascal, SI unit)
14:31, 5 October 2008Thumbnail for version as of 14:31, 5 October 20083,000 × 1,934 (59 KB)Ruslik0{{Information |Description={{en|1=The image shows the vertical strusture of the atmosphere of Jupiter. The temperature is show as function of pressure (black line). The approximate altitudes of transitions troposhere–stratopshere (tropopause) and st

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